Photometry of asteroids (5141), (43032), (85953), (259221), and (363599) observed at Pic du Midi Observatory

These are the first results of an observational program devoted to the complete physical data of asteroids that could produce or feed meteoroid streams. Our results are based on the optical observation at Pic du Midi observatory in April 6–7, 2016 and January 17–18, 2018. We will present the light c...

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Bibliographic Details
Published inAstronomische Nachrichten Vol. 339; no. 2-3; pp. 198 - 203
Main Authors Dumitru, B. A., Birlan, M., Sonka, A., Colas, F., Nedelcu, D. A.
Format Journal Article
LanguageEnglish
Published Weinheim WILEY‐VCH Verlag GmbH & Co. KGaA 01.02.2018
Wiley Subscription Services, Inc
Wiley-VCH Verlag
Subjects
Asteroids
Astrophysics
colors
Daytime
Light curve
near earth asteroids
NEAs
Observatories
Photometry
Physics
Pic du Midi
Pic du Midi
asteroids
near earth asteroids
photometry
NEAs
colors
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Summary:These are the first results of an observational program devoted to the complete physical data of asteroids that could produce or feed meteoroid streams. Our results are based on the optical observation at Pic du Midi observatory in April 6–7, 2016 and January 17–18, 2018. We will present the light curve of asteroid (259221) 2003 BA21, associated with Daytime Sextantids (221 DSX) and November θ Aurigids (390 THA); the light curves and colors of asteroid (363599) 2004 FG11, associated with Daytime ζ Perseids (172 ZPE) as well as g − r and g − i; and the corresponding reflectances for the (85953) 1999 FK21, associated with Daytime ξ Sagittariids (100 XSA). We will also present the colors for two additional objects, namely, (5141) Tachibana and (43032) 1999 VR26.
ISSN:0004-6337
1521-3994
DOI:10.1002/asna.201813463